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Weighing the Invisible

Section 4 of 11

The Rotation-Curve Surprise

Part 3: The Rotation-Curve Surprise

Now move from the central black hole to the entire disk of a galaxy. The Solar System gives us a useful expectation. Nearly all of the Solar System’s mass is in the Sun. As you move outward, the enclosed mass barely changes, so the orbital speed decreases with distance.

You can see that directly from the same equation. Solving for the speed gives . For the Solar System outside the Sun the enclosed mass is approximately constant, , so and therefore . In a central-mass system, larger-radius orbits move more slowly.

Teaching plot showing that orbital speed decreases with distance in the Solar System because the Sun contains nearly all of the enclosed mass.
Figure 7What to notice: in a central-mass system like the Solar System, orbital speed falls with distance. This is the prediction that fails for the outer parts of spiral galaxies.Course illustration (A. Rosen)

That falling curve is what we would expect if most of a galaxy’s mass were concentrated where most of its light is. Spiral galaxies have bright stellar disks. If the visible disk contained most of the mass, then stars and gas far from the center should orbit more slowly, much like outer planets orbit the Sun more slowly than inner planets.

Three side-by-side model rotation curves comparing a central mass system, a visible disk only model, and a disk plus dark halo model with high outer orbital speeds.
Figure 8What to notice: a central mass gives falling speeds, visible matter alone cannot sustain high outer speeds, and adding an extended halo produces the approximately flat outer rotation curve we observe.Course illustration (A. Rosen)

But that is not what we observe.

Plot of the Milky Way rotation curve showing orbital speed versus distance from the Galactic center, with data points remaining high at large radii compared with a declining luminous-matter expectation.
Figure 9What to notice: the Milky Way's rotation curve stays roughly flat instead of falling like a Solar-System curve. The simplest inference is that mass keeps increasing with radius even where there is little visible light.

The Milky Way’s rotation curve stays roughly flat over a large range of radius. Gas and stars far from the Galactic center orbit faster than the visible matter alone would predict. The simplest interpretation is that the enclosed mass keeps increasing with radius, even where the visible light becomes faint.

Rotation curve

A plot of orbital speed versus distance from the center of a galaxy. Its shape encodes how mass is distributed: a falling curve means a central mass concentration; a flat curve means mass that keeps growing outward.

Here the word “flat” needs careful math grammar. A flat rotation curve means the speed is approximately constant, . Put that into the enclosed-mass scaling : if is approximately constant, then is too, so . The speed curve is flat, but the enclosed-mass curve rises.

Flat rotation curve

A galaxy rotation curve in which orbital speed stays roughly constant with radius. Through , a flat speed implies an enclosed mass that rises in proportion to radius — the signature of an extended dark-matter halo.

Two-panel teaching plot. The top panel shows orbital speed staying nearly constant with radius, while the bottom panel shows enclosed mass rising with radius for the same flat speed curve.
Figure 10What to notice: a flat speed curve is not a flat mass curve. If orbital speed stays approximately constant while radius increases, then the enclosed mass must keep rising roughly in proportion to radius.Course illustration (A. Rosen)

External galaxies show the same pattern.

Plot of the rotation curve for galaxy UGC 11455, with observed speeds at large radius exceeding the curve expected from visible components alone.
Figure 11What to notice: external galaxy rotation curves show the same pattern: measured speeds remain high far from the bright disk. This makes dark matter a population-level inference, not a one-galaxy oddity.

This matters because it turns dark matter from a one-galaxy oddity into a population-level inference. If many spiral galaxies show flat rotation curves, then the problem is not that we made one bad map of the Milky Way. The pattern is telling us something general about galaxy mass distributions.

Diagram comparing an observed flat galaxy rotation curve with an expected declining curve from observed luminosity, overlaid on an image of a spiral galaxy.
Figure 12What to notice: the observed rotation curve stays flat while the curve predicted from visible matter declines. The gap is the evidence a dark matter halo is meant to explain.

The term dark matter is a name for the inferred gravitating component that does not emit, absorb, or scatter enough light for us to see directly. The word “dark” does not mean mysterious magic. It means electromagnetically dark: visible through gravity, not through ordinary light. We infer it because the gravitational model requires more mass than the luminous matter provides.

Dark matter

A gravitating component inferred from motion, lensing, and structure formation that does not emit, absorb, or scatter enough light to be seen directly. “Dark” means electromagnetically dark — visible through gravity, not through ordinary light. This reading, built on rotation curves and the Bullet Cluster, is its canonical home in the course.

Multiple choice

If a spiral galaxy has a flat rotation curve far beyond its bright stellar disk, what is the most direct inference from ?

Quick check

Suppose a galaxy’s rotation speed stays about constant as radius doubles. According to , what happens to the enclosed mass?